Figure 2 from Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections

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Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections

Authors: Julián D. Alvarado-Gómez, Jeremy J. Drake, Federico Fraschetti, Cecilia Garraffo, Ofer Cohen, Christian Vocks, Katja Poppenhäger, Sofia P. Moschou, Rakesh K. Yadav, and Ward B. Manchester IV

2020 The Astrophysical Journal 895 47.

Provider: AAS Journals

Caption: Figure 2.

Radial profiles of V_A extracted from each of the AWSoM steady-state solutions (Figure 1, white lines). Active region (AR) and coronal hole (CH) profiles are included for the solar case (top panel). Four latitudes are probed in our two stellar cases (middle and bottom panels). The stellar wind speed (V^SW) along each profile is indicated by the color scale.

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